Supernova 1993J in M81
Spanish
Version
INTRODUCTION.
SN 1993J appeared in NGC 3031 (M81) , a galaxy located in Ursa Major ,
12 m.l.y. far away from us, has been one of the brightest an best studied
SNe of the modern Astronomy.
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It has been the brightest SN appeared in the northern Hemisphere in the
latest 21 years.
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This is probably the SN with a more exact knowledge about the right moment
of the explosion.
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It has been monitored and studied by the most sophisticated professional
telescopes, this includes Hubble, M. palomar , Roque de los Muchachos ,
and VLA telescopes, and Rosat , Asca, IUE.... Satellites..
SN 1993J was discovered on the 28th of March , Sunday night , By Francisco
Garcia Díaz , amateur astronomer living in Lugo , Spain with a 10"
telescope. Francisco is an active member of M1.
This group was created five years ago by M.A.A. members Diego Rodriguez
, José Ripero and Francisco Pujol. Since the very begining we were
aware that to find a SN was an extremely difficult task, but there was
Robert Evans example , amateurs astronomer with 26 discoveries . This fact
encouraged us to keep observing and try to find a new small point not included
in the M. Palomar images or in the Thompson Bryan charts.
The group gathered botch , equipment and bibliography to do SN hunting
( RealSky Thompson-Bryan charts , CCD Buil-Thouvenot , and Lopez Alvarez
Atlases, etc...) We also own a computer program able to provide asteroid
appulses to deep-sky objects , and therefore , to clarify possible false
alarms due to asteroids.
Francisco Garcia , joined the group three years ago. In the five years
prior to the discovery we achieved 25.000 negative observations checking
650 different galaxies . We have also been able to observe and monitor
visually , photographically and with CCD , SN 1989 in M66 , (This SN was
one of the reasons to create the group ), SN 1991T in NGC 4527 , SN 1991X
in NGC 4902 and SN 1992G in NGC 3294.
Chronology of the discovery of SN 1993J in M 81
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Sunday, 28th of March 1993
Francisco García , member of the SN Search Group M1 , observed a
suspected star in the galaxy NGC 3031 (M81) , located in Ursa Major , He
estimated it to be m=11.8 . He called inmediately Jose Carvajal , M1 member
also , asking him to verify in the Asteroids Appulses computer program
, whether there was an asteroid.While Francisco Observes again the galaxy
, Jose Carvajal calls Diego Rodriguez, another M1 members , asking him
to take a CCD image of the galaxy and thus , to confirm that the suspected
new star was present. In that position nothing appeared in the Thonson
Bryan , Buil-Thouvenot and Hubble Atlases. Diego Rodriguez called Enrique
Pérez, Spanish astronomer astronomer observing that night with 2.5
meters aperture Issaac Newton Telescope , in the Roque de los Muchachos
Observatory in Canary Island. Enrique replied he was not sure whether he
would be able to confirm the SN .
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Monday, 29th of March 1993
The twilight of Monday 29th , found Diego Rodriguez , Francisco Pujol ,
Francisco Garcia , and José Ripero , waiting anxiously , the first
star of the night to confirm the suspected new SN... Actually , the star
was in the same position and showed a brightness of m=11 , estimations
were made both , visually and with CCD .
After this confirmation we called urgently Dr. Wamsteker , Scientific Director
of VILSPA , we also sent him by Fax a copy of the CCD image taken by Diego
Rodriguez. Afterwards we called Janet Mattei (AAVSO) to confirm the SN
. Finally we talked to our good Australian Friend Rovert Evans the amateur
with more SNe decoveries. In the same night , a few hours late , the first
spectrum of the SN was taken by Enrique Pérez in the 2.5 meters
aperture Isaac Newton Telescope.
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Wednesday, 31th of March 1993
Early in the morning we received , at last , The IAU Circular 5731 announcing
the discovery of SN 1993J by Francisco Garcia -Diaz of Lugo Spain , and
the SN group M1 of Madrid Astronomical Association. El PAIS , the most
important Spanish newspaper , covers the information , and remarks the
importance of this event discovered by Madrid amateurs astronomers.
Important highlights of this covery
There are a few aspects to be pointed out related to this discovery:
1.-The very short time that elapsed between the visual discovery and the
CCD image.This became crucial to know the exact SN position , and thus
, to make easier the spectral confirmation by professional telescopes.
2.- We were also very fast confirming this was neither an asteroid , nor
a variable star lurking near the galaxy, Just a few minutes after the first
sight , it had already been confirmed by another observer.
3.- A second visual confirmation , performed 24h later by most M1 members
definitely assured this star was a real SN.
4.- All this was possible due to the existence of an organized team with
good experience and resources to go ahead without doubst in case a SN arises.
Importance and peculiarities of SN 1993J
The following reasons make SN 1993J very peculiar:
This SN appeared in very close galaxy . Whit the exception of SN 1987A
, found in the Large Magellenic Cloud , modern Astronomy has never aimed
its telescopes to a so near SN.
The explosion time is known with just a few hours of uncertainty . Actually
, there is a photographic observation performed on saturday ,27th of March
, at 21h45 (UT) . In the picture take by the French amateur J.C. Merlin
, nothing brigther than m=16 appeared in the SN position .
On Sunday 28th of March , A.W. Neely , American amateur took some CCD images
at 7h15 (UT) . At this time the SN was already present and showed a brightness
of m=13.7 .
On Sunday 28th of March , at 21h45 (UT) , Francisco Garcia made discovery
and estimated the SN to be at m=11.8
According to last news sent By Dr. de Vaucouleurs , professional astronomers
consider explosion began on the midday of saturday 27th of March. This
assumption is based on theoretical models about the evolution of the SN
brightness . For this calculation it is assumed that the initial brightness
of the progenitor
star should be m=20.8
SN 1993J showed twon maximum
of light. The first happened one day after the discovery , while the second
one occurred three weeks later.
A nearly unique spectral behaviour . SN 1987K appeared in NGC 4651 (Virgo)
, and SN 1993J in M81 , are the only ones that moved from type II when
the explosion , to type Ib , some time later . Therefore , SN 1993J represents
a repetition of very unusual behaviour.
SN 1987K was discovered by Berkeley Automated SN Search Group , led by
Pennypacker , in late July 1987 ; this SN achieved m=14.2 . Based on its
spectrum , it was initially classified as type II (plateau) to a type Ib
. Actually , in the spectrum taken on May 11 1993 , all alfa hydrogen lines
had vanished . According to Astrophysic theories , wide and clear oxigen
an calcium lines will fill the spectrum in the coming weeks.
Progenitor star mass has been estimated to be in the rage of 10-20 M.O.
recognitions.
To Dr. Wilhem Wamsteker , Director of Villafranca Tracking Station, (VILSPA),
and to all his team.
To Mrs. Janet Mattei , AAVSO Director , she helped us a lot spreading through
electronic-mails the new of our discovery to most Observatories and Universities.
To SNe Group ,of IAC (Intituto Astrofisica de Canarias), conducted by Dr
. Mr. Francisco Sánchez , and specially to Mr . Gaby Gómez
, member of this group , for the continuous information provided about
the behaviour of SN 1993J.
To all wives , mothers, girlfriens , sons and daughters ... of M1 group
members , to bear our madness until the new about the discovery arrived
. And obviously , to share their lives with us and with SN 1993J . We are
in debit for your understanding and help...
SN 1993J Light curve.
The
Progenitor of SN 1993J
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Principal/Return.
Actualizado el 5 de Mayo de 1997
M-1